Beyond Caustic Crossings: Properties of Binary Microlensing Light Curves
Abstract
Binary microlensing light curves have a variety of morphologies. Many are indistinguishable from point-lens light curves. Of those that deviate from the point-lens form, caustic crossing light curves have tended to dominate identified binary-lens events. Other distinctive signatures of binary lenses include significant asymmetry, multiple peaks, and repeating events. We have quantified, using high-resolution simulations, the theoretically expected relative numbers of each type of binary-lens event, based on its measurable characteristics. We find that a microlensing survey with current levels of photometric uncertainty and sampling should contain at least as many non-caustic crossing binary-lens events as caustic crossing events; in future surveys with more sensitive photometry, the contribution of distinctive non-caustic crossing events will be even greater. To show that this result is robust, we investigate the influence of several physical effects, including blending, sampling rate, and various binary populations.
Additional Information
© 2008 The American Astronomical Society. Received 2007 April 24; accepted 2008 May 19. R. D. would like to thank Rosalba Perna and Nada Petrovic for conversations. Funded in part by NASA NAG5-10705, PHY05- 51164, and a grant for SAO Internal Research and Development.Attached Files
Published - NIGapj08.pdf
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Additional details
- Eprint ID
- 13520
- Resolver ID
- CaltechAUTHORS:NIGapj08
- NASA
- NAG5-10705
- NASA
- PHY05-51164
- SAO Internal Research and Development
- Created
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2009-07-17Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field